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Some Anticipated SolarCISM
"Products"
- New "rules of thumb" for
coronal mass ejection predictions,
based on CME modeling.
- Web-accessible Time series of simulated solar wind
MHD variables (velocity, density/dynamic pressure,
vector magnetic field) at 1 AU
- Simulated white-light coronal images and
coronal hole boundaries from the global MHD
coronal model, available at a web site
- Solar energetic particle event predictions
based on magnetic connectivity of earth to
the Sun
- Selected solar XUV flux estimates based on photospheric
magnetic field observations
- Educational webpages
to show how we make models
from solar observations, and
how the models can be used to make predictions
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